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20032026
most citedDynamical age differences among coeval star clusters as revealed by blue stragglers

216 citations · 1.7k across the 41 of their papers we have counts for

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Showing 2019Show all

10 papers · 1 filter

astro-ph.SR201918 cited

A study of the blue straggler population of the old open cluster Collinder 261

M. J. Rain, G. Carraro, J. A. Ahumada +4

Blue Stragglers are stars located in an unexpected region of the color-magnitude diagram of a stellar population, as they appear bluer and more luminous than the stars in the turno…

astro-ph.GA20197 cited

The Smallest Scale of Hierarchy Survey (SSH). I. Survey Description

F. Annibali, G. Beccari, M. Bellazzini +7

The Smallest Scale of Hierarchy (SSH) survey is an ongoing strategic large program at the Large Binocular Telescope, aimed at the detection of faint stellar streams and satellites…

astro-ph.SR201948 cited

Uncovering a 260 pc wide, 35 Myr old filamentary relic of star formation

Giacomo Beccari, Henri M. J. Boffin, Tereza Jerabkova

Several recent studies have shown that the Vela OB2 region hosts a complex constellation of sub-populations with ages in the range 10 to 50 Myr. Such populations might represent th…

astro-ph.GA201930 cited

Star density profiles of six old star clusters in the Large Magellanic Cloud

B. Lanzoni, F. R. Ferraro, E. Dalessandro +7

We used resolved star counts from Hubble Space Telescope images to determine the center of gravity and the projected density profiles of 6 old globular clusters in the Large Magell…

astro-ph.SR2019

A stellar relic filament in the Orion star forming region

Tereza Jerabkova, Henri M. J. Boffin, Giacomo Beccari +1

We report the discovery of the oldest stellar substructure in the Orion star forming region (OSFR), the Orion relic filament. The relic filament is physically associated with the O…

astro-ph.GA2019

Size diversity of old Large Magellanic Cloud clusters as determined by internal dynamical evolution

F. R. Ferraro, B. Lanzoni, E. Dalessandro +6

The distribution of size as a function of age observed for star clusters in the Large Magellanic Cloud (LMC) is very puzzling: young clusters are all compact, while the oldest syst…